Quantum imprints of gravitational shockwaves
Abstract Gravitational shockwaves are simple exact solutions of Einstein equations representing the fields of ultrarelativistic sources and idealized gravitational waves (shocks). Historically, much work has focused on shockwaves in the context of possible black hole formation in high energy particl...
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oai:doaj.org-article:5ccd1b9141be442a9950dc313718730a2021-11-14T12:41:19ZQuantum imprints of gravitational shockwaves10.1007/JHEP11(2021)0541029-8479https://doaj.org/article/5ccd1b9141be442a9950dc313718730a2021-11-01T00:00:00Zhttps://doi.org/10.1007/JHEP11(2021)054https://doaj.org/toc/1029-8479Abstract Gravitational shockwaves are simple exact solutions of Einstein equations representing the fields of ultrarelativistic sources and idealized gravitational waves (shocks). Historically, much work has focused on shockwaves in the context of possible black hole formation in high energy particle collisions, yet they remain at the forefront of research even today. Representing hard modes in the bulk, shocks give rise to the gravitational memory effect at the classical level and implant supertranslation (BMS) hair onto a classical spacetime at the quantum level. The aim of this paper is to further our understanding of the ‘information content’ of such supertranslations. Namely, we show that, contrary to the several claims in the literature, a gravitational shockwave does leave a quantum imprint on the vacuum state of a test quantum field and that this imprint is accessible to local observers carrying Unruh-DeWitt (UDW) detectors in this spacetime.Finnian GrayDavid KubizňákTaillte MaySydney TimmermanErickson TjoaSpringerOpenarticleClassical Theories of GravityGauge SymmetrySpace-Time SymmetriesNuclear and particle physics. Atomic energy. RadioactivityQC770-798ENJournal of High Energy Physics, Vol 2021, Iss 11, Pp 1-32 (2021) |
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Classical Theories of Gravity Gauge Symmetry Space-Time Symmetries Nuclear and particle physics. Atomic energy. Radioactivity QC770-798 |
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Classical Theories of Gravity Gauge Symmetry Space-Time Symmetries Nuclear and particle physics. Atomic energy. Radioactivity QC770-798 Finnian Gray David Kubizňák Taillte May Sydney Timmerman Erickson Tjoa Quantum imprints of gravitational shockwaves |
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Abstract Gravitational shockwaves are simple exact solutions of Einstein equations representing the fields of ultrarelativistic sources and idealized gravitational waves (shocks). Historically, much work has focused on shockwaves in the context of possible black hole formation in high energy particle collisions, yet they remain at the forefront of research even today. Representing hard modes in the bulk, shocks give rise to the gravitational memory effect at the classical level and implant supertranslation (BMS) hair onto a classical spacetime at the quantum level. The aim of this paper is to further our understanding of the ‘information content’ of such supertranslations. Namely, we show that, contrary to the several claims in the literature, a gravitational shockwave does leave a quantum imprint on the vacuum state of a test quantum field and that this imprint is accessible to local observers carrying Unruh-DeWitt (UDW) detectors in this spacetime. |
format |
article |
author |
Finnian Gray David Kubizňák Taillte May Sydney Timmerman Erickson Tjoa |
author_facet |
Finnian Gray David Kubizňák Taillte May Sydney Timmerman Erickson Tjoa |
author_sort |
Finnian Gray |
title |
Quantum imprints of gravitational shockwaves |
title_short |
Quantum imprints of gravitational shockwaves |
title_full |
Quantum imprints of gravitational shockwaves |
title_fullStr |
Quantum imprints of gravitational shockwaves |
title_full_unstemmed |
Quantum imprints of gravitational shockwaves |
title_sort |
quantum imprints of gravitational shockwaves |
publisher |
SpringerOpen |
publishDate |
2021 |
url |
https://doaj.org/article/5ccd1b9141be442a9950dc313718730a |
work_keys_str_mv |
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1718429050166312960 |